All Tables

Table 2: The parameters of the Gaussian components of the [OIII] lines. Gaussian widths (W) and $\Delta z= z_{\rm NLR2}-z_{\rm NLR1}$ are given in km s^-1. The intensity ratio $R_{\rm NLR1}=I_{5007}/I_{4959}$ of the "blue component'' obtained from the Gaussian fit, the measured flux ratio $R_{\rm F}=F_{5007}/F_{4959}$ and central intensity ratio of the "blue'' and "central'' Gaussian components ( $I_{\rm B}/I_{\rm C}$ ) are also given (Cols. 2, 3 and 6). The data for the objects denoted with stars should be taken with caution, because their [OIII] lines are too weak.
Table 3: The parameters of the disk: $z_{\rm l}$ is the shift and $W_{\rm l}=\sqrt {2}\sigma$ is the Gaussian broadening term from the disk which is a measure of the random velocity in the disk, $R_{\rm inn}$ is the inner radius, $R_{\rm out}$ is the outer radius. $z_{\rm G}$ and $W_{\rm G}$ represent the parameters of the Gaussian component.
Table 1: The observed AGNs with the coordinates, redshift, central wavelength and exposition.